Summary Page for Probing dark energy using the X-ray gas mass fraction in dynamically relaxed galaxy clusters
Probing dark energy using the X-ray gas mass fraction in dynamically relaxed galaxy clusters

Target: Abell 2029

Chandra
X-ray
Center

PI: Dr Steven Allen 
Seq Num: 800549
Obs ID: 6101
Instrument: ACIS




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Full Field with Sources
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Full Field with Sources
Full Field with Sources



List of the Brighest Sources in the Field
RA[deg] DEC[deg] NET_COUNTS[count] NET_COUNTS_ERR[count] SNR
227.776648 5.689666 518.511353 24.681902 21.007755
227.890407 5.763206 103.458336 12.825927 8.066343
227.890314 5.763106 100.193184 12.573394 7.968667
227.655255 5.803735 73.055176 10.783501 6.774718
227.751966 5.820110 33.714287 7.591296 4.441177
227.831598 5.860272 24.958334 6.629393 3.764799
227.864240 5.662029 31.666666 8.456709 3.744561
227.751731 5.822462 23.142857 7.317101 3.162845
227.885342 5.690387 21.833334 7.004494 3.117046
227.749397 5.751587 18.000000 5.845194 3.079453


Postscript Summary Page